BY Alec Marshak & Kyle Harding

Slides:



Advertisements
Similar presentations
Motions of the Planets This presentation will introduce these terms: Geocentric, Heliocentric, Retrograde, Rotation, Revolution.
Advertisements

A circle is tangent to the x-axis at (-2, 0) and the y-axis at (0, 2). What is the equation of this circle?
Copyright © Cengage Learning. All rights reserved. Conic Sections.
Lab Practical Information Regents Earth Science When? Wednesday 5/31/2011 –Everyone.
Why does eccentricity only vary between 0 and 1?
Regents Exam Lab Practical Review.
Conic sections project
 Period of Rotation: The amount of time it takes for a planet to make one spin around its imaginary axis  Period of rotation determines the length of.
The Solar System Planetary Orbits
Ellipses. Solve each equation = x x 2 = = 120 – x 2 Ellipses - Warm Up.
Planetary Orbits The ancient Greeks (Aristotle and Plato) thought the only perfect shapes were the circle and line. All things fall in a line toward Earth,
Warm Up Find the distance between (0, -2) & (4, 3)
To our science fair project On ASTRONOMY SCIENCE.
What is rotation? Spinning on an imaginary axis Period of rotation is the time it takes for a planet to make 1 spin on its axis =length of a planet day.
O RBIT OF M ERCURY ASTR 110G Section M09 September 30 th, 2010
Copyright © Cengage Learning. All rights reserved. 9.2 Ellipses.
Ellipses. Ellipse An ellipse is a closed curve around two fixed points called foci. Earth, and all the planets, revolve around (orbit) the sun in an eccentric,
Kepler’s Laws of Planetary Motion © David Hoult 2009.
Kepler’s Laws of Planetary Motion STARTER 2 In an elliptical planetary orbit, the sun is a. at the center of the ellipse. b. on the ellipse at the intersection.
Geometry of Earth’s Orbit Kepler’s Laws of Planetary Motion.
 Ms. Susinno’s Earth Science Class. The scandalous life of Tycho Brahe.
 Danish astronomer ( )  Built an astronomical observatory on an island  Measured positions of stars and planets over a period of 20 years.
Eccentricity. Definition Degree of ovalness of an orbit around the sun.
10.3 Ellipses Foci Major Axis / Minor Axis Vertices / Co- Vertices Eccentricity.
Accelerated Precalculus Ellipses. One Minute Question Find the diameter of: x 2 + y 2 + 6x - 14y + 9 = 0.
10.3 ELLIPSES Write equations of ellipses in standard form and graph ellipses. Use properties of ellipses to model and solve real-life problems. Find eccentricities.
Orbit of Mercury Yeah protractors!. Planetary Orbits - All planets orbit the Sun in an ellipse - Semi-major axis (a) is half of the long axis.
Eccentricity.
Aristotle suggested an Earth-centered, or geocentric, model of the solar system. In this model, the sun, the stars, an the planets revolved around Earth.
Conics Name the vertex and the distance from the vertex to the focus of the equation (y+4) 2 = -16(x-1) Question:
Orbits, Asteroids, and Comets. The Geometry of Orbits Planets revolve in an ellipse around the sun –An ellipse has two fixed points called foci that are.
“Kepler’s” Laws of Orbital motion
Splash Screen.
Our Solar System.
Aim: How do we calculate the eccentricity of an ellipse?
Write a polar equation in r and {image} of a parabola with the focus at the origin and directrix x = {image}
Orbits and Eccentricity
Kepler’s Laws of Planetary Motion
ASTR 110G Section M09 September 30th, 2010
Day 1.
It’s gonna get eccentric…
Science Starter Kepler’s 1st law states that planetary orbits are _________________ shapes? Kepler’s 2nd law states that 2 equal intervals of time an imaginary.
THE.
foci {image} None of these choices
I’m pumped for this part of the Regents!
Section 2: Models of the Solar System
Conic Sections Ellipse The Sequal.
Our Solar System ©Mark Place,
Models of the Solar System
Lesson 9.2 Ellipses.
Lab Practical Information
Physics of the Solar System
Section 2: Models of the Solar System
Copyright © Cengage Learning. All rights reserved.
Which planet has the most eccentric orbit?
Lesson 2 Models of the Universe
Lab Practical Review Day 2
Kepler’s Laws of Planetary Motion
September 12 – 16, 2011 Welcome Assignment
10.4 Ellipses Elliptical Orbits Elliptical Galaxies
Aim: How can we explain the laws that control the planets orbits?
Eccentricity.
Aim: How do we compute Eccentricity?
QQ: Name the planets in our Solar System in order moving away from the Sun. What is the largest planet? What is the smallest planet? Which planet is closest.
U5D2 Assignment, pencil, red pen, highlighter, calculator, notebook
10.3 Ellipses.
M3CSD2 Have out: Bellwork:
Eccentricity.
Kepler’s Laws of Planetary Motion
Motion of Objects in Space
Presentation transcript:

BY Alec Marshak & Kyle Harding Making an ellipse BY Alec Marshak & Kyle Harding

Supplies Two pushpins A piece of computer paper A big piece of cardboard A 20cm long piece of string that is tied together to form a loop Lastly you need a pencil

Steps # 1-3 First fold the paper in half like a hot dog then open it and place it on the cardboard Now draw two dots that are two centimeters apart in the middle of the paper Now label the left focus F1 and the right focus F2 (The Sun)

Steps #4-7 Place the pushpins into the two dots. Make sure to have pushed the pushpins all the way into the cardboard Now you will put the string around the pushpins and insert your pencil inside the string loop Use it by drawing a circle while puling outward on the string with your pencil (make sure the string stays on the pins)

Congratulations Steps 7-8 Take out the pushpins Now draw a straight line through the middle of the ellipse connecting the foci to the outside of the ellipse and label it the major axis Lastly, hand the perfect ellipse to your Earth Science teacher and hope for the best Congratulations

Finding the Eccentricity When finding the eccentricity of an ellipse, you use the equation e=d/l . e=eccentricity, d=distance between foci, and l=length of major axis. So the steps are… Measure the distance between the foci.(cm) Measure the length of the major axis.(cm) Divide the distance between the foci by the length of the major axis and the answer is the eccentricity.(cm to the nearest thousandth)

Our Ellipse So using the steps from the last slide, we will figure out our ellipse’s eccentricity. The d=2 cm and the l= 10.8 cm.Next we divide 2cm by 10.8cm which equals .185.So our ellipse has an eccentricity of .185. Now that we know our ellipse’s eccentricity we can compare it to another planet’s eccentricity. Compared to Mercury’s eccentricity our planet’s eccentricity is less eccentric. If our ellipse was a planet’s orbit, and it was compared to Mercury’s orbit our planet’s orbit would be less than and more circular.